The Integrated Global Geodetic Observing System (IGGOS) viewed from the perspective of history

Towards the end of the 19th century, geodetic observation techniques allowed it to create geodetic networks of continental size. The insight that big networks can only be set up through international collaboration led to the establishment of an international collaboration called “Central European Arc Measurement”, the predecessor of the International Association of Geodesy (IAG), in 1864. The scope of IAG activities was extended already in the 19th century to include gravity.At the same time, astrometric observations could be made with an accuracy of a few tenths of an arcsecond. The accuracy stayed roughly on this level, till the space age opened the door for milliarcsecond (mas) astrometry. Astrometric observations allowed it at the end of the 19th century to prove the existence of polar motion. The insight that polar motion is almost unpredictable led to the establishment of the International Latitude Service (ILS) in 1899.The IAG and the ILS were the tools (a) to establish and maintain the terrestrial and the celestial reference systems, including the transformation parameters between the two systems, and (b) to determine the Earth's gravity field.Satellite-geodetic techniques and astrometric radio-interferometric techniques revolutionized geodesy in the second half of the 20th century. Satellite Laser Ranging (SLR) and methods based on the interferometric exploitation of microwave signals (stemming from Quasars and/or from satellites) allow it to realize the celestial reference frame with (sub-)mas accuracy, the global terrestrial reference frame with (sub-)cm accuracy, and to monitor the transformation between the systems with a high time resolution and (sub-)mas accuracy. This development led to the replacement of the ILS through the IERS, the International Earth Rotation Service in 1989.In the pre-space era, the Earth's gravity field could “only” be established by terrestrial methods. The determination of the Earth's gravitational field was revolutionized twice in the space era, first by observing geodetic satellites with optical, Laser, and Doppler techniques, secondly by implementing a continuous tracking with spaceborne GPS receivers in connection with satellite gradiometry. The sequence of the satellite gravity missions CHAMP, GRACE, and GOCE allow it to name the first decade of the 21st century the “decade of gravity field determination”.The techniques to establish and monitor the geometric and gravimetric reference frames are about to reach a mature state and will be the prevailing geodetic tools of the following decades. It is our duty to work in the spirit of our forefathers by creating similarly stable organizations within IAG with the declared goal to produce the geometric and gravimetric reference frames (including their time evolution) with the best available techniques and to make accurate and consistent products available to wider Earth sciences community as a basis for meaningful research in global change. IGGOS, the Integrated Global Geodetic Observing System, is IAG's attempt to achieve these goals. It is based on the well-functioning and well-established network of IAG services.     

根据IGRF计算1995～2000年中国及邻区地磁长期变化

根据最新的第七代国际地磁参考场,计算并绘制１９９５～２０００年中国及邻区地磁长期变化图,分析了长期变化的空间变化。     

ECMWF参考大气谱模式在Convex320机上的发展

将ＥＣＭＷＦ预报模式移植到Ｃｏｎｖｅｘ３２０机上，修改了Ｉ／Ｏ结构，使得该模式在该机上顺利运行，在模式中引入了参考大气。计算了６个实例，取得了较好的结果，另外，在该模式上还ＣＸＳ格式，节省了计算时间，也提高了计算精度。     

太阳系质心参考系与地心参考系中的激光测距问题

给出了太阳系质心参考系（BRS）和地心参考系（GRS）中的相对论激光测距理论模型,并且利用现有的坐标变换关系证明两种模型在毫米级的精度上是完全等价的。最后指出,由IERS推荐的坐标变换公式与激光测距模型之间存在不自洽性,这种不自恰性对激光测月（LLR）的影响可达约10cm。     

地心非旋转坐标系中卫星共视法时间比对计算模型

卫星导航定位系统测距的基础是测时,定轨和定位的前提是各观测量的时间同步,因此,时间同步技术是卫星导航定位系统建设的关键技术基础之一。卫星导航定位系统中时间同步技术包括卫星与地面（星-地）和地面站间（地-地）的时间同步。在本文中,根据卫星共视法时间比对的基本原理,分别从数学角度和几何角度详细推导了地心非旋转坐标系中卫星共视法时间比对的基本计算模型,从而为实现站间高精度的时间同步提供了一些参考。     

基于多参考站网络的VRS算法研究与实现

多参考站网络的建立,为网络RTK的实现奠定了基础。虚拟参考站技术是网络RTK的一种,它以众多的优势代表了网络RTK的主要发展趋势。简单介绍了VRS系统的工作原理;从基准站间双差改正数的生成、虚拟观测值的生成和流动站处的定位解算3个方面,详细推导了VRS的数学模型;针对差分改正信息,提出了综合误差内插算法;最后,利用4个已知点的观测数据,结合编程计算,证明了文中VRS数学模型的正确性,为虚拟参考站系统的进一步研究提供依据。     

基于约束三维重力反演的南极大陆地壳密度结构研究

地壳密度是表征其物质组成以及结构特征的一个基本参数,是深入理解构造演化、地球动力学等问题的重要基础.本文利用最新发布的布格重力异常数据,以现有的三维S波速度模型、地表热流以及岩石学数据作为约束条件,采用引入深度加权函数的三维重力反演算法,获取了南极大陆三维精细密度结构模型.研究结果显示,南极大陆地壳尺度范围内密度异常在-0.25～0.20g·cm^-3之间.大致以南极横断山脉为界,受中生代与新生代多期拉张活动的影响,西南极上地壳密度异常以低值为主,与东南极克拉通的高密度异常呈现明显对比关系.通过对比发现,反演的密度结构与岩石圈强度信息存在较好的相关性.进一步分析西南极裂谷系统的密度结构与岩石圈强度,认为受新生代拉张活动和岩浆活动影响的局部地区除外,热沉降作用很可能使得地壳趋于冷却.此外,西南极的低密度特征延伸到南极横断山脉,结合现有的研究结果认为可能需要多种机制来解释南极横断山脉的隆升过程.     

CHAMP型卫星定轨顾及非线性改正的轨道扰动方程

本文针对CHAMP型卫星建立了顾及非线性改正的轨道扰动方程定轨理论与方法.首先从卫星运动的二阶微分方程出发,引入了正常引力位以及相应的参考轨道,然后分别推导了线性化轨道扰动方程与顾及非线性改正的轨道扰动方程,同时说明了建立的线性化轨道扰动方程与目前处理CHAMP卫星数据的动力学定轨方法是等价的.其次分别对线性化轨道扰动方程与顾及非线性改正的轨道扰动方程的精度进行了估计,在卫星定位精度为3cm与非惯性力测量精度为3×10~(-10)m·s~(-2)的前提下证明了下列结论:当参考轨道与实际轨道之间的距离ρ≤4.7m时线性化轨道扰动方程的精度能达到非惯性力的测量精度以及当ρ≤4.14×10~3m时顾及非线性改正的轨道扰动方程能达到非惯性力的测量精度.由此便可得出结论:相对于线性化轨道扰动方程,顾及非线性改正的轨道扰动方程具有更高的精度,且适合在更长的时间弧段上建立关于引力场位系数的法方程组,特别是针对CHAMP卫星计划进行的模拟计算也完全验证了该结论.最后利用叠加原理,给出了顾及非线性改正的轨道扰动方程的求解方法.此外,还针对GRACE卫星计划利用顾及非线性改正的轨道扰动方程进行了恢复引力场的模拟计算,结果表明:分段建立位系数的法方程组时子弧段分别取值2h、1d、6 d对恢复引力场的结果几乎不产生影响,这表明在处理GRACE数据时能够以6d的弧长来建立法方程组.     

Correction of apparent position shifts caused by GNSS antenna changes

Antenna changes at GNSS reference stations frequently produce discontinuities in the coordinate time series. These apparent position shifts are mainly caused by changes of carrier-phase multipath effects and different errors in the antenna phase center corrections. A monitoring method was developed and successfully tested, which requires additional GNSS observations from a local, temporary reference station. Changes of carrier-phase measurement errors due to the antenna change are determined and stored in L1 and L2 phase maps. These phase maps provide corrections to be applied either to the observation data obtained before the antenna change or to the observation data obtained after the antenna change. The observation corrections are able to remove coordinate discontinuities independent of the selected coordinate estimation algorithm.

K-Ar法地质年龄标准物质ZBJ角闪石的定值结果

为了满足K-Ar定年中K和⁴⁰Ar^*分析的质量监控及Ar-Ar法样品在反应堆照射时中子通量监测的需要,我国氩同位素年代学工作者研制了一个K-Ar法年龄标准物质ZBJ角闪石,它采自北京房山花岗闪长岩体。它的⁴⁰Ar-³⁹Ar阶段加热分析结果表明:⁴⁰Ar^*在矿物晶格中保存均匀稳定,年龄谱平坦,³⁹Ar析出量高达97%。这些证据充分表明该黑云母结晶以后未受过热扰动,40K-⁴⁰Ar^*同位素计时体系封闭良好。坪年龄为133.3±0.6Ma,总气体年龄为134.4±1.4Ma,³⁶Ar/⁴⁰Ar-³⁹Ar/⁴⁰Ar反等时线年龄为133.2±0.8Ma,⁴⁰Ar/³⁶Ar初始值为297.6±4.8,此值与(⁴⁰Ar/³⁶Ar)a大气氩丰度比(295.5±0.5)处于同一范围,表明样品不含过剩氩。这几个年龄值的一致性,说明该样品具有良好的均匀性和稳定性,它作为K-Ar和Ar-Ar法地质年龄标准物质是适合的。ZBJ角闪石均匀性检验结果表明:在0.05显著性水平下经统计学方法检验,证明K和⁴⁰Ar^*的F分布值小于F临界值,说明该样品是均匀的。国内8个实验室参加了ZBJ角闪石K含量和⁴⁰Ar^*含量的定值分析,经统计学方法检验,结果显示全部定值数据都服从正态分布并具等精度。在置信概率为0.95时,⁴⁰Ar*和K含量的相对标准偏差都小于1%。两个特性量值定值分析结果的一致值(认定值)和不确定度分别为:⁴⁰Ar^*=(2.464±0.018)×10^-10mol/g,K=(1.027±0.008)%,K-Ar年龄(标准值)=133.3±1.5Ma(2σ)。此标准物质纯度为98.1%,粒度为0.15～0.30mm,总重量为740g,缩分成最小样品单元共100瓶,每瓶7.4g,可供我国K-Ar和Ar-Ar法同位素年代学实验室使用37年。